Numerical study of rotating relativistic stars

Thumbnail image of item number 1 in: 'Numerical study of rotating relativistic stars'.
Thumbnail image of item number 2 in: 'Numerical study of rotating relativistic stars'.
Thumbnail image of item number 3 in: 'Numerical study of rotating relativistic stars'.
Thumbnail image of item number 4 in: 'Numerical study of rotating relativistic stars'.
Showing 1-4 of 55 pages in this article.

PDF Version Also Available for Download.

Description

The equations of structure for rotating stars in general relativity are presented and put in a form suitable for computer calculations. The results of equilibrium calculations for supermassive stars, neutron stars, and magnetically supported stars are reported, as are calculations of collapsing, rotating, and magnetized stars in the slowly changing gravitational field approximation. (auth)

Physical Description

Pages: 54

Creation Information

Wilson, J.R. August 25, 1975.

Context

This article is part of the collection entitled: Office of Scientific & Technical Information Technical Reports and was provided by UNT Libraries Government Documents Department to Digital Library, a digital repository hosted by the UNT Libraries. More information about this article can be viewed below.

Who

People and organizations associated with either the creation of this article or its content.

Author

Publisher

Provided By

UNT Libraries Government Documents Department

Serving as both a federal and a state depository library, the UNT Libraries Government Documents Department maintains millions of items in a variety of formats. The department is a member of the FDLP Content Partnerships Program and an Affiliated Archive of the National Archives.

About | Browse this Partner

Contact Us

Corrections Questions

What

Descriptive information to help identify this article. Follow the links below to find similar items on the Digital Library.

Description

The equations of structure for rotating stars in general relativity are presented and put in a form suitable for computer calculations. The results of equilibrium calculations for supermassive stars, neutron stars, and magnetically supported stars are reported, as are calculations of collapsing, rotating, and magnetized stars in the slowly changing gravitational field approximation. (auth)

Physical Description

Pages: 54

Notes

Dep. NTIS

Source

  • Meeting of physics and astrophysics of neutron stars and black holes, Varenna, Italy, 14 Jul 1975

Language

Item Type

Identifier

Unique identifying numbers for this article in the Digital Library or other systems.

  • Report No.: UCRL--76967
  • Report No.: CONF-750744--1
  • Grant Number: None
  • Office of Scientific & Technical Information Report Number: 4199816
  • Archival Resource Key: ark:/67531/metadc878022

Collections

This article is part of the following collection of related materials.

Office of Scientific & Technical Information Technical Reports

Reports, articles and other documents harvested from the Office of Scientific and Technical Information.

Office of Scientific and Technical Information (OSTI) is the Department of Energy (DOE) office that collects, preserves, and disseminates DOE-sponsored research and development (R&D) results that are the outcomes of R&D projects or other funded activities at DOE labs and facilities nationwide and grantees at universities and other institutions.

About | Browse this Collection

What responsibilities do I have when using this article?

Digital Files

When

Dates and time periods associated with this article.

Creation Date

  • August 25, 1975

Added to The UNT Digital Library

  • Sept. 21, 2016, 2:29 a.m.

Description Last Updated

  • Oct. 18, 2016, 1:54 p.m.

Usage Statistics

When was this article last used?

Yesterday: 0
Past 30 days: 0
Total Uses: 3
More Statistics

Interact With This Article

Here are some suggestions for what to do next.

Start Reading

Thumbnail image of item number 1 in: 'Numerical study of rotating relativistic stars'.
Thumbnail image of item number 2 in: 'Numerical study of rotating relativistic stars'.
Thumbnail image of item number 3 in: 'Numerical study of rotating relativistic stars'.
Thumbnail image of item number 4 in: 'Numerical study of rotating relativistic stars'.

PDF Version Also Available for Download.

Citations, Rights, Re-Use

Wilson, J.R. Numerical study of rotating relativistic stars, article, August 25, 1975; Livermore, California. (digital.library.unt.edu/ark:/67531/metadc878022/: accessed April 24, 2018), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT Libraries Government Documents Department.